Contains:  Solar system body or event
A Negative spoked Lunar Craters, Astroavani - Avani Soares

A Negative spoked Lunar Craters

A Negative spoked Lunar Craters, Astroavani - Avani Soares

A Negative spoked Lunar Craters

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Description

The image below shows a reverse view of the Moon which highlights the visibility of bright ray craters. As shown here, most large rayed craters of the visible side of the Moon are near the lunar equator, Langrenus, Copernicus and Kepler. The crater Tycho is a big exception, as well as others that are clustered around the north polar region. A negative view as it calls attention to the rays that have their source crater as yet uncertain. The Bessel beam that crosses the Mare Serenitatis is a famous example. It can come from Tycho, but no other ray of Tycho comes so far from their source. It may come from the coast of Menelaus Serenitatis, but why the hell would reach this go so far? Fainter rays crossing the Imbrium could also long rays of Tycho, but they are not radial to that crater and are usually parallel to each other rather than diverge. This view also shows the distribution of the rays of Tycho. It is well known that some of the rays of Tycho extend westward, but here we can also see that some rays follow to southeast, with two exceptions towards the pole. The image below, like many other imagnes Moon, raise good questions that encourages us to ever want to study more and more our only natural satellite, the Moon

Text taken from "Rubens Center for the Study of the Moon"

GSO 12 "+ Fuji compact camera + 25mm KK ortho

Photo in afocal and single exposure.

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A Negative spoked Lunar Craters, Astroavani - Avani Soares